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Introduction to GRB Physics
- Long GRBs: core collapse of rapidly rotating, stripped massive stars forming a black hole or magnetar, launching relativistic jets through the stellar envelope.
- Short GRBs: mergers of neutron star–neutron star or neutron star–black hole binaries producing a short-lived accreting black hole or hypermassive neutron star, again launching jets. The engine must produce collimated, high-Lorentz-factor (Γ ≳ 100) outflows to avoid pair-production opacity that would otherwise thermalize gamma rays.
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